Published April 1, 2021 | Version Accepted Version + Published
Journal Article Open

Topological superconductivity in nanowires proximate to a diffusive superconductor–magnetic-insulator bilayer

  • 1. ROR icon University of California, Santa Barbara
  • 2. ROR icon California Institute of Technology
  • 3. ROR icon Massachusetts Institute of Technology
  • 4. ROR icon Microsoft (United States)

Abstract

We study semiconductor nanowires coupled to a bilayer of a disordered superconductor and a magnetic insulator, motivated by recent experiments reporting possible Majorana-zero-mode signatures in related architectures. Specifically, we pursue a quasiclassical Usadel equation approach that treats superconductivity in the bilayer self-consistently in the presence of spin-orbit scattering, magnetic-impurity scattering, and Zeeman splitting induced by both the magnetic insulator and a supplemental applied field. Within this framework we explore prospects for engineering topological superconductivity in a nanowire proximate to the bilayer. We find that a magnetic-insulator-induced Zeeman splitting, mediated through the superconductor alone, cannot induce a topological phase since the destruction of superconductivity (i.e., Clogston limit) preempts the required regime in which the nanowire's Zeeman energy exceeds the induced pairing strength. However, this Zeeman splitting does reduce the critical applied field needed to access the topological phase transition, with fields antiparallel to the magnetization of the magnetic insulator having an optimal effect. Finally, we show that magnetic-impurity scattering degrades the topological phase, and spin-orbit scattering, if present in the superconductor, pushes the Clogston limit to higher fields yet simultaneously increases the critical applied field strength.

Additional Information

© 2021 American Physical Society. Received 15 January 2021; revised 5 March 2021; accepted 8 March 2021; published 7 April 2021. We thank Bela Bauer, Roman Lutchyn, Saulius Vaitiekėnas, Charles M. Marcus, Chun-Xiao Liu, Michael Wimmer, and Chetan Nayak for useful discussions. A.K. also thanks Matthew P. A. Fisher and Andrea F. Young for valuable comments. P.A.L. acknowledges support from the NSF C-Accel Track C Grant No. 2040620. J.A.'s work was supported by Army Research Office under Grant Award No. W911NF17-1-0323; the National Science Foundation through Grant No. DMR-1723367; the Caltech Institute for Quantum Information and Matter, an NSF Physics Frontiers Center with support of the Gordon and Betty Moore Foundation through Grant No. GBMF1250; and the Walter Burke Institute for Theoretical Physics at Caltech. The final stage of this work was in part based on support by the U.S. Department of Energy, Office of Science through the Quantum Science Center (QSC), a National Quantum Information Science Research Center. A.K.'s work was supported by Microsoft corporation. Use was made of computational facilities purchased with funds from the National Science Foundation (Grant No. CNS-1725797) and administered by the Center for Scientific Computing (CSC). The CSC is supported by the California NanoSystems Institute and the Materials Research Science and Engineering Center (MRSEC; Grant No. NSF DMR 1720256) at UC Santa Barbara.

Attached Files

Published - PhysRevB.103.134506.pdf

Accepted Version - 2012.12934.pdf

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2012.12934.pdf

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Additional details

Identifiers

Eprint ID
108784
Resolver ID
CaltechAUTHORS:20210421-103423569

Related works

Funding

NSF
OIA-2040620
Army Research Office (ARO)
W911NF17-1-0323
NSF
DMR-1723367
Institute for Quantum Information and Matter (IQIM)
Gordon and Betty Moore Foundation
GBMF1250
Walter Burke Institute for Theoretical Physics, Caltech
Department of Energy (DOE)
Microsoft Corporation
NSF
CNS-1725797
California NanoSystems Institute
NSF
DMR-1720256

Dates

Created
2021-04-21
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Updated
2021-04-21
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